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Spectroscopy: the key to the stars
This is the first non-technical book on spectroscopy written specifically for practical amateur astronomers. It includes all the science necessary for a qualitative understanding of stellar spectra, but avoids a mathematical treatment which would alienate many of its intended readers. Any amateur as...
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Lenguaje: | eng |
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Springer
2007
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Acceso en línea: | https://dx.doi.org/10.1007/978-0-387-68288-4 http://cds.cern.ch/record/1621311 |
_version_ | 1780933186023325696 |
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author | Robinson, Keith |
author_facet | Robinson, Keith |
author_sort | Robinson, Keith |
collection | CERN |
description | This is the first non-technical book on spectroscopy written specifically for practical amateur astronomers. It includes all the science necessary for a qualitative understanding of stellar spectra, but avoids a mathematical treatment which would alienate many of its intended readers. Any amateur astronomer who carries out observational spectroscopy and who wants a non-technical account of the physical processes which determine the intensity and profile morphology of lines in stellar spectra will find this is the only book written specially for them. It is an ideal companion to existing books |
id | cern-1621311 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2007 |
publisher | Springer |
record_format | invenio |
spelling | cern-16213112021-04-21T21:51:21Zdoi:10.1007/978-0-387-68288-4http://cds.cern.ch/record/1621311engRobinson, KeithSpectroscopy: the key to the starsAstrophysics and AstronomyThis is the first non-technical book on spectroscopy written specifically for practical amateur astronomers. It includes all the science necessary for a qualitative understanding of stellar spectra, but avoids a mathematical treatment which would alienate many of its intended readers. Any amateur astronomer who carries out observational spectroscopy and who wants a non-technical account of the physical processes which determine the intensity and profile morphology of lines in stellar spectra will find this is the only book written specially for them. It is an ideal companion to existing books Springeroai:cds.cern.ch:16213112007 |
spellingShingle | Astrophysics and Astronomy Robinson, Keith Spectroscopy: the key to the stars |
title | Spectroscopy: the key to the stars |
title_full | Spectroscopy: the key to the stars |
title_fullStr | Spectroscopy: the key to the stars |
title_full_unstemmed | Spectroscopy: the key to the stars |
title_short | Spectroscopy: the key to the stars |
title_sort | spectroscopy: the key to the stars |
topic | Astrophysics and Astronomy |
url | https://dx.doi.org/10.1007/978-0-387-68288-4 http://cds.cern.ch/record/1621311 |
work_keys_str_mv | AT robinsonkeith spectroscopythekeytothestars |